Search Publications

ARES. II. Characterizing the Hot Jupiters WASP-127 b, WASP-79 b, and WASP-62b with the Hubble Space Telescope
DOI: 10.3847/1538-3881/ab94a3 Bibcode: 2020AJ....160..109S

Drossart, Pierre; Blain, Doriann; Beaulieu, Jean-Philippe +24 more

This paper presents the atmospheric characterization of three large, gaseous planets: WASP-127 b, WASP-79 b, and WASP-62 b. We analyzed spectroscopic data obtained with the G141 grism (1.088-1.68 µm) of the Wide Field Camera 3 on board the Hubble Space Telescope using the Iraclis pipeline and the TauREx3 retrieval code, both of which are pub…

2020 The Astronomical Journal
eHST 73
Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in the SPTpol 100-square-degree Survey
DOI: 10.3847/1538-3881/ab6a96 Bibcode: 2020AJ....159..110H

Sharon, K.; Gladders, M. D.; Ade, P. A. R. +74 more

We present a catalog of galaxy cluster candidates detected in 100 square degrees surveyed with the SPTpol receiver on the South Pole Telescope. The catalog contains 89 candidates detected with a signal-to-noise ratio greater than 4.6. The candidates are selected using the Sunyaev-Zel'dovich effect at 95 and 150 GHz. Using both space- and ground-ba…

2020 The Astronomical Journal
Gaia 69
Accretion Properties of PDS 70b with MUSE
DOI: 10.3847/1538-3881/ab811e Bibcode: 2020AJ....159..222H

Uyama, Taichi; Takasao, Shinsuke; Hashimoto, Jun +4 more

We report a new evaluation of the accretion properties of PDS 70b obtained with the Very Large Telescope/Multi Unit Spectroscopic Explorer. The main difference from the previous studies of Haffert et al. and Aoyama & Ikoma is in the mass accretion rate. Simultaneous multiple line observations, such as Hα and Hβ, can better constrain the physic…

2020 The Astronomical Journal
Gaia 68
Mitigation of LEO Satellite Brightness and Trail Effects on the Rubin Observatory LSST
DOI: 10.3847/1538-3881/abba3e Bibcode: 2020AJ....160..226T

Yoachim, Peter; Tyson, J. Anthony; Ivezić, Željko +8 more

We report studies on the mitigation of optical effects of bright low-Earth-orbit (LEO) satellites on Vera C. Rubin Observatory and its Legacy Survey of Space and Time (LSST). These include options for pointing the telescope to avoid satellites, laboratory investigations of bright trails on the Rubin Observatory LSST camera sensors, algorithms for …

2020 The Astronomical Journal
Gaia 67
The High-energy Radiation Environment around a 10 Gyr M Dwarf: Habitable at Last?
DOI: 10.3847/1538-3881/abb465 Bibcode: 2020AJ....160..237F

Loyd, R. O. Parke; Kowalski, Adam F.; Brown, Alexander +20 more

Recent work has demonstrated that high levels of X-ray and UV activity on young M dwarfs may drive rapid atmospheric escape on temperate, terrestrial planets orbiting within the habitable zone. However, secondary atmospheres on planets orbiting older, less active M dwarfs may be stable and present more promising candidates for biomarker searches. …

2020 The Astronomical Journal
eHST 65
Observations of Disequilibrium CO Chemistry in the Coldest Brown Dwarfs
DOI: 10.3847/1538-3881/ab9114 Bibcode: 2020AJ....160...63M

Fortney, Jonathan J.; Marley, Mark S.; Freedman, Richard S. +10 more

Cold brown dwarfs are excellent analogs of widely separated, gas giant exoplanets, and provide insight into the potential atmospheric chemistry and physics we may encounter in objects to be discovered by future direct imaging surveys. We present a low-resolution, R ∼ 300, M-band spectroscopic sequence of seven brown dwarfs with effective temperatu…

2020 The Astronomical Journal
ISO 65
The Hawaii Infrared Parallax Program. IV. A Comprehensive Parallax Survey of L0-T8 Dwarfs with UKIRT
DOI: 10.3847/1538-3881/ab84f4 Bibcode: 2020AJ....159..257B

Magnier, Eugene A.; Dupuy, Trent J.; Liu, Michael C. +1 more

We present parallaxes, proper motions, and J-band photometry for 348 L and T dwarfs measured using the wide-field near-infrared camera WFCAM on the United Kingdom Infrared Telescope. This is the largest single batch of infrared parallaxes for brown dwarfs to date. Our parallaxes have a median uncertainty of 3.5 mas, similar to most previous ground…

2020 The Astronomical Journal
Gaia 63
A Sub-Neptune-sized Planet Transiting the M2.5 Dwarf G 9-40: Validation with the Habitable-zone Planet Finder
DOI: 10.3847/1538-3881/ab5f15 Bibcode: 2020AJ....159..100S

Endl, Michael; Mahadevan, Suvrath; Terrien, Ryan +32 more

We validate the discovery of a 2-Earth-radii sub-Neptune-sized planet around the nearby high-proper-motion M2.5 dwarf G 9-40 (EPIC 212048748), using high-precision, near-infrared (NIR) radial velocity (RV) observations with the Habitable-zone Planet Finder (HPF), precision diffuser-assisted ground-based photometry with a custom narrowband photomet…

2020 The Astronomical Journal
Gaia 63
A Dynamical Mass of 70 ± 5 MJup for Gliese 229B, the First T Dwarf
DOI: 10.3847/1538-3881/abb45e Bibcode: 2020AJ....160..196B

Dupuy, Trent J.; Bardalez Gagliuffi, Daniella C.; Bowler, Brendan P. +4 more

We combine Keck/HIRES radial velocities, imaging with HiCIAO/Subaru and the Hubble Space Telescope, and absolute astrometry from Hipparcos and Gaia to measure a dynamical mass of 70 ± 5 ${M}_{\mathrm{Jup}}$ for the brown dwarf companion to Gl 229. Gl 229B was the first imaged brown dwarf to show clear signs of methane in its atmosphere. Cooling mo…

2020 The Astronomical Journal
Gaia Hipparcos eHST 62
Occurrence and Architecture of Kepler Planetary Systems as Functions of Stellar Mass and Effective Temperature
DOI: 10.3847/1538-3881/ab7373 Bibcode: 2020AJ....159..164Y

Zhou, Ji-Lin; Xie, Ji-Wei; Yang, Jia-Yi

The Kepler mission has discovered thousands of exoplanets around various stars with different spectral types (M, K, G, and F) and thus different masses and effective temperatures. Previous studies have shown that the planet occurrence rate, in terms of the average number of planets per star, drops with increasing stellar effective temperature (T

2020 The Astronomical Journal
Gaia 61